Timing of 29 Pulsars Discovered in the PALFA SurveyCitation formats

  • External authors:
  • A.~G. Lyne
  • S. Bogdanov
  • R.~D. Ferdman
  • P.~C.~C. Freire
  • V.~M. Kaspi
  • B. Knispel
  • R. Lynch
  • B. Allen
  • A. Brazier
  • F. Camilo
  • F. Cardoso
  • S. Chatterjee
  • J.~M. Cordes
  • F. Crawford
  • J.~S. Deneva
  • J.~W.~T. Hessels
  • F.~A. Jenet
  • P. Lazarus
  • J. van Leeuwen
  • D.~R. Lorimer
  • E. Madsen
  • J. McKee
  • M.~A. McLaughlin
  • E. Parent
  • C. Patel
  • S.~M. Ransom
  • P. Scholz
  • A. Seymour
  • X. Siemens
  • L.~G. Spitler
  • I.~H. Stairs
  • K. Stovall
  • J. Swiggum
  • R.~S. Wharton
  • W.~W. Zhu
  • C. Aulbert
  • O. Bock
  • H.-B. Eggenstein
  • H. Fehrmann
  • B. Machenschalk

Standard

Timing of 29 Pulsars Discovered in the PALFA Survey. / Lyne, A.~G.; Stappers, B.~W.; Bogdanov, S.; Ferdman, R.~D.; Freire, P.~C.~C.; Kaspi, V.~M.; Knispel, B.; Lynch, R.; Allen, B.; Brazier, A.; Camilo, F.; Cardoso, F.; Chatterjee, S.; Cordes, J.~M.; Crawford, F.; Deneva, J.~S.; Hessels, J.~W.~T.; Jenet, F.~A.; Lazarus, P.; van Leeuwen, J.; Lorimer, D.~R.; Madsen, E.; McKee, J.; McLaughlin, M.~A.; Parent, E.; Patel, C.; Ransom, S.~M.; Scholz, P.; Seymour, A.; Siemens, X.; Spitler, L.~G.; Stairs, I.~H.; Stovall, K.; Swiggum, J.; Wharton, R.~S.; Zhu, W.~W.; Aulbert, C.; Bock, O.; Eggenstein, H.-B.; Fehrmann, H.; Machenschalk, B.

In: The Astrophysical Journal, Vol. 834, 01.01.2017, p. 137.

Research output: Contribution to journalArticlepeer-review

Harvard

Lyne, AG, Stappers, BW, Bogdanov, S, Ferdman, RD, Freire, PCC, Kaspi, VM, Knispel, B, Lynch, R, Allen, B, Brazier, A, Camilo, F, Cardoso, F, Chatterjee, S, Cordes, JM, Crawford, F, Deneva, JS, Hessels, JWT, Jenet, FA, Lazarus, P, van Leeuwen, J, Lorimer, DR, Madsen, E, McKee, J, McLaughlin, MA, Parent, E, Patel, C, Ransom, SM, Scholz, P, Seymour, A, Siemens, X, Spitler, LG, Stairs, IH, Stovall, K, Swiggum, J, Wharton, RS, Zhu, WW, Aulbert, C, Bock, O, Eggenstein, H-B, Fehrmann, H & Machenschalk, B 2017, 'Timing of 29 Pulsars Discovered in the PALFA Survey', The Astrophysical Journal, vol. 834, pp. 137. https://doi.org/10.3847/1538-4357/834/2/137

APA

Lyne, A. G., Stappers, B. W., Bogdanov, S., Ferdman, R. D., Freire, P. C. C., Kaspi, V. M., Knispel, B., Lynch, R., Allen, B., Brazier, A., Camilo, F., Cardoso, F., Chatterjee, S., Cordes, J. M., Crawford, F., Deneva, J. S., Hessels, J. W. T., Jenet, F. A., Lazarus, P., ... Machenschalk, B. (2017). Timing of 29 Pulsars Discovered in the PALFA Survey. The Astrophysical Journal, 834, 137. https://doi.org/10.3847/1538-4357/834/2/137

Vancouver

Lyne AG, Stappers BW, Bogdanov S, Ferdman RD, Freire PCC, Kaspi VM et al. Timing of 29 Pulsars Discovered in the PALFA Survey. The Astrophysical Journal. 2017 Jan 1;834:137. https://doi.org/10.3847/1538-4357/834/2/137

Author

Lyne, A.~G. ; Stappers, B.~W. ; Bogdanov, S. ; Ferdman, R.~D. ; Freire, P.~C.~C. ; Kaspi, V.~M. ; Knispel, B. ; Lynch, R. ; Allen, B. ; Brazier, A. ; Camilo, F. ; Cardoso, F. ; Chatterjee, S. ; Cordes, J.~M. ; Crawford, F. ; Deneva, J.~S. ; Hessels, J.~W.~T. ; Jenet, F.~A. ; Lazarus, P. ; van Leeuwen, J. ; Lorimer, D.~R. ; Madsen, E. ; McKee, J. ; McLaughlin, M.~A. ; Parent, E. ; Patel, C. ; Ransom, S.~M. ; Scholz, P. ; Seymour, A. ; Siemens, X. ; Spitler, L.~G. ; Stairs, I.~H. ; Stovall, K. ; Swiggum, J. ; Wharton, R.~S. ; Zhu, W.~W. ; Aulbert, C. ; Bock, O. ; Eggenstein, H.-B. ; Fehrmann, H. ; Machenschalk, B. / Timing of 29 Pulsars Discovered in the PALFA Survey. In: The Astrophysical Journal. 2017 ; Vol. 834. pp. 137.

Bibtex

@article{7c542fa7bbdf47e3a64efaff90aaa945,
title = "Timing of 29 Pulsars Discovered in the PALFA Survey",
abstract = "We report on the discovery and timing observations of 29 distant long-period pulsars discovered in the ongoing Arecibo PALFA pulsar survey. Following discovery with the Arecibo Telescope, conrmation and timing observations of these pulsars over several years at Jodrell Bank Observatory have yielded high-precision positions and measurements of rotation and radiation properties. We have used multi-frequency data to measure the interstellar scattering properties of some of these pulsars. Most of the pulsars have properties that mirror those of the previously known pulsar population, although four show some notable characteristics. PSRs J1907+0631 and J1925+1720 are young and are associated with supernova remnants or plerionic nebulae: J1907+0631 lies close to the center of SNR G40.5􀀀0.5, while J1925+1720 is coincident with a high-energyFermi -ray source. One pulsar, J1932+1500, is in a surprisingly eccentric, 199-day binary orbit with a companion having a minimum mass of 0.33 M. Several of the sources exhibit timing noise, and two, PSRs J0611+1436 and J1907+0631, have both suered large glitches, but with very dierent post-glitch rotation properties. In particular, the rotational period of PSR J0611+1436 will not recover to its pre-glitch value for about 12 years, a far greater recovery timescale than seen following any other large glitches.",
keywords = "pulsars: general, pulsars: individual: PSR J0611+1436, PSR J1907+0631, PSR J1925+1720, PSR J1932+1500",
author = "A.~G. Lyne and B.~W. Stappers and S. Bogdanov and R.~D. Ferdman and P.~C.~C. Freire and V.~M. Kaspi and B. Knispel and R. Lynch and B. Allen and A. Brazier and F. Camilo and F. Cardoso and S. Chatterjee and J.~M. Cordes and F. Crawford and J.~S. Deneva and J.~W.~T. Hessels and F.~A. Jenet and P. Lazarus and {van Leeuwen}, J. and D.~R. Lorimer and E. Madsen and J. McKee and M.~A. McLaughlin and E. Parent and C. Patel and S.~M. Ransom and P. Scholz and A. Seymour and X. Siemens and L.~G. Spitler and I.~H. Stairs and K. Stovall and J. Swiggum and R.~S. Wharton and W.~W. Zhu and C. Aulbert and O. Bock and H.-B. Eggenstein and H. Fehrmann and B. Machenschalk",
year = "2017",
month = jan,
day = "1",
doi = "10.3847/1538-4357/834/2/137",
language = "English",
volume = "834",
pages = "137",
journal = "The Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",

}

RIS

TY - JOUR

T1 - Timing of 29 Pulsars Discovered in the PALFA Survey

AU - Lyne, A.~G.

AU - Stappers, B.~W.

AU - Bogdanov, S.

AU - Ferdman, R.~D.

AU - Freire, P.~C.~C.

AU - Kaspi, V.~M.

AU - Knispel, B.

AU - Lynch, R.

AU - Allen, B.

AU - Brazier, A.

AU - Camilo, F.

AU - Cardoso, F.

AU - Chatterjee, S.

AU - Cordes, J.~M.

AU - Crawford, F.

AU - Deneva, J.~S.

AU - Hessels, J.~W.~T.

AU - Jenet, F.~A.

AU - Lazarus, P.

AU - van Leeuwen, J.

AU - Lorimer, D.~R.

AU - Madsen, E.

AU - McKee, J.

AU - McLaughlin, M.~A.

AU - Parent, E.

AU - Patel, C.

AU - Ransom, S.~M.

AU - Scholz, P.

AU - Seymour, A.

AU - Siemens, X.

AU - Spitler, L.~G.

AU - Stairs, I.~H.

AU - Stovall, K.

AU - Swiggum, J.

AU - Wharton, R.~S.

AU - Zhu, W.~W.

AU - Aulbert, C.

AU - Bock, O.

AU - Eggenstein, H.-B.

AU - Fehrmann, H.

AU - Machenschalk, B.

PY - 2017/1/1

Y1 - 2017/1/1

N2 - We report on the discovery and timing observations of 29 distant long-period pulsars discovered in the ongoing Arecibo PALFA pulsar survey. Following discovery with the Arecibo Telescope, conrmation and timing observations of these pulsars over several years at Jodrell Bank Observatory have yielded high-precision positions and measurements of rotation and radiation properties. We have used multi-frequency data to measure the interstellar scattering properties of some of these pulsars. Most of the pulsars have properties that mirror those of the previously known pulsar population, although four show some notable characteristics. PSRs J1907+0631 and J1925+1720 are young and are associated with supernova remnants or plerionic nebulae: J1907+0631 lies close to the center of SNR G40.5􀀀0.5, while J1925+1720 is coincident with a high-energyFermi -ray source. One pulsar, J1932+1500, is in a surprisingly eccentric, 199-day binary orbit with a companion having a minimum mass of 0.33 M. Several of the sources exhibit timing noise, and two, PSRs J0611+1436 and J1907+0631, have both suered large glitches, but with very dierent post-glitch rotation properties. In particular, the rotational period of PSR J0611+1436 will not recover to its pre-glitch value for about 12 years, a far greater recovery timescale than seen following any other large glitches.

AB - We report on the discovery and timing observations of 29 distant long-period pulsars discovered in the ongoing Arecibo PALFA pulsar survey. Following discovery with the Arecibo Telescope, conrmation and timing observations of these pulsars over several years at Jodrell Bank Observatory have yielded high-precision positions and measurements of rotation and radiation properties. We have used multi-frequency data to measure the interstellar scattering properties of some of these pulsars. Most of the pulsars have properties that mirror those of the previously known pulsar population, although four show some notable characteristics. PSRs J1907+0631 and J1925+1720 are young and are associated with supernova remnants or plerionic nebulae: J1907+0631 lies close to the center of SNR G40.5􀀀0.5, while J1925+1720 is coincident with a high-energyFermi -ray source. One pulsar, J1932+1500, is in a surprisingly eccentric, 199-day binary orbit with a companion having a minimum mass of 0.33 M. Several of the sources exhibit timing noise, and two, PSRs J0611+1436 and J1907+0631, have both suered large glitches, but with very dierent post-glitch rotation properties. In particular, the rotational period of PSR J0611+1436 will not recover to its pre-glitch value for about 12 years, a far greater recovery timescale than seen following any other large glitches.

KW - pulsars: general, pulsars: individual: PSR J0611+1436, PSR J1907+0631, PSR J1925+1720, PSR J1932+1500

U2 - 10.3847/1538-4357/834/2/137

DO - 10.3847/1538-4357/834/2/137

M3 - Article

VL - 834

SP - 137

JO - The Astrophysical Journal

JF - The Astrophysical Journal

SN - 0004-637X

ER -